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The relative f-values for 63 lines in 17 multiplets of Tin in the wave-length range XX 3143-3761 have been measured. The method was essentially that described in Mt. W. Conir. Nos. 528 and 581, with the exception that a high-pressure mercury arc was used as the source of the continuous spectrum, thus enabling furnace absorption lines to be observed at temperatures up to 30000 C
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Robert B. King (1941) studied this question.
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